The geomagnetic field was quiet on February 7. Solar wind speed
ranged between 312 and 378 km/s.

Solar flux measured at 20h UTC on 2.8 GHz was 90.3. The planetary A index was
3 (STAR Ap - based on the mean of three hour interval ap
indices: 2.8). Three hour interval K indices: 10000112 (planetary),
11101122 (Boulder).

The background x-ray flux is at the class B4 level.

At midnight there were 2 spotted regions on the visible solar disk.

Region 11045 added many spots and more than doubled its penumbral
area. The first magnetic delta structure weakened after the M6 event, however, a
new delta structure has formed further east and the region remains capable of
producing further major flares and Earth directed CMEs. Flares:
A major M6.4/1N flare was recorded at
02:34 UTC. This event was associated with a CME which very likely will impact Earth, probably on February 9.
Other flares: C1.1 at 03:29, C9.9/1F at 04:52, C4.2 at 21:15, C4.2 at 21:39 and
C1.0 at 22:31 UTC.
New region 11046 emerged near the northeast limb.

February 5: No obvious partially or fully Earth directed CMEs were observed in LASCO
or STEREO imagery.February 6: A CME was observed off of the east limb after an M2 flare in region 11045.February 7: A full halo CME was observed following an M6 flare in region 11045.

A recurrent coronal hole (CH390) in the northern hemisphere was in
an Earth facing position on February 6-7. A coronal hole (CH391) in the southern
hemisphere could reach an Earth facing position on February 8.

Processed SOHO/EIT 195 image at 23:48 UTC on February 7. The darkest areas on the solar disk are likely coronal holes.

Long distance low and medium
frequency (below 2 MHz) propagation
along paths north of due west over high and upper middle latitudes is fair. Propagation on long distance northeast-southwest paths
is poor.

The geomagnetic field is expected to be quiet to unsettled on February 8. The CME
associated with the major flare in region 11045 on Feb.7 could impact Earth on February 9
and cause unsettled to major storm conditions. A high
speed stream from CH390 could cause unsettled to active conditions on February
10.

Coronal holes (1)

Coronal mass ejections (2)

M and X class flares (3)

1) Effects from a coronal hole could reach Earth
within the next 5 days. When the high speed stream has arrived the
color changes to green.
2) Effects from a CME are likely to be observed at Earth within 96 hours.
3) There is a possibility of either M or X class flares within the next 48 hours.

Data for all numbered solar regions according to the Solar Region
Summary provided by NOAA/SWPC. Comments are my own, as is the
STAR spot count (spots observed at or inside a few hours before
midnight) and data for regions not numbered by SWPC or where SWPC has observed no spots.
SWPC active region numbers in the table below and in the active region
map above are the historic SWPC/USAF numbers.

1) Running average based on the
daily 20:00 UTC observed solar flux
value at 2800 MHz.
2) Unofficial, accumulated value based on the Boulder (NOAA/SWPC) sunspot number. The official international sunspot number is typically
30-50% lower.
3) Running average based on the
daily SWPC ap indices. Values in red are based on
official NGDC records.

This report has been prepared by Jan
Alvestad. It is based partly on my own observations and analysis,
and
partly on data from some of these solar data sources.
All time references are to the UTC day. Comments and suggestions are
always welcome.